Abstract
AbstractWe recently studied the energy behavior of a quantum‐corrected time‐dependent black hole. The system analyzed was a quantum‐corrected Kerr solution that settles down to a stationary configuration as the time dependence fades out. A trans‐Planckian energy scaling in the vicinity of the event horizon resulted, and we proposed the trans‐Planckian radiation to be the missing link in the glowing mechanism of active galactic nuclei. The main goal of the present work is to examine the scaling and structure of the radiation by analyzing the quantum momentum density. We again observe a trans‐Planckian behavior. Furthermore, the momentum density displays structures that are indicative of a disk‐like configuration near the equator and a collimated outflow of matter from the poles. The bipolar outflow (disk‐like structure) should be an essential part of the underlying mechanism for jets (accretion disks) of active galactic nuclei.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
